Searches for solar axions have been carried out with
various experimental techniques: magnetic helioscopes
[1]}, [2]}, low temperature bolometers [3]}
and thin foil nuclear targets [4]}.
CUORE(Cryogenic Underground
Observatory for Rare Events) [5]}, [6]}, [7]}, [8]}, [9]} as well as
the Majorana Demonstrator [10]} which are designed to search for neutrinoless double beta
decay (\(0\nu \beta \beta \) ) using very low background detectors
are used for the axion searches. The Ge detectors in GERDA
[11]} can also be used to search for dark matter weakly
interacting massive particles (WIMPs) and axion searches
[12]}, [13]}, [14]}.
